Figure 17 from Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves

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Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves

Authors: Yan-Fei Jiang (姜燕飞), Paul J. Green, Jenny E. Greene, Eric Morganson, Yue Shen, Anna Pancoast, Chelsea L. MacLeod, Scott F. Anderson, W. N. Brandt, C. J. Grier, H.-W. Rix, John J. Ruan, Pavlos Protopapas, Caroline Scott, W. S. Burgett, K. W. Hodapp, M. E. Huber, N. Kaiser, R. P. Kudritzki, E. A. Magnier, N. Metcalfe, J. T. Tonry, R. J. Wainscoat, and C. Waters

2017 The Astrophysical Journal 836 186.

Provider: AAS Journals

Caption: Figure 17.

Top: summary of the stacked lag signals with median luminosity for the whole sample. The open black, red, and blue triangles are the stacked g − r, g − i, and g − z lags as shown in Figure 10. The filled black, red, and blue circles are the stacked g − r, g − i, and g − z lags for two luminosity bins with the theoretically expected values for each luminosity bin connected by the black, red, and blue lines. Bottom: the corresponding stacked lags of the subsample cLD for two luminosity bins as shown in Figure 13.

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